N. Blackaby et al., THE NONLINEAR EVOLUTION OF INVISCID GORTLER VORTICES IN 3-DIMENSIONALBOUNDARY-LAYERS, Philosophical transactions-Royal Society of London. Physical sciences and engineering, 355(1726), 1997, pp. 975-1016
The nonlinear development of inviscid Gortler vortices in a three-dime
nsional boundary-layer flow is considered by extending the theory of B
lackaby et al., who consider the closely related problem concerning th
e nonlinear development of disturbances in stratified shear flows. The
inviscid Gortler modes considered are initially unstable (and hence g
rowing) based on linear theory; however, following others, we assume t
hat the effects of boundary-layer spreading result in them evolving in
a linear fashion until they reach a stage where their amplitudes are
sufficiently large, and their growth rates have diminished sufficientl
y, such that their subsequent evolution can be considered within the f
ramework of a weakly nonlinear theory based on a nonlinear, non-equili
brium critical-layer theory. As with the closely related stratified-sh
ear flow problem, three possible nonlinear integro-differential evolut
ion equations for the disturbance amplitude should arise: however, it
is found that only two of these are in fact possible. One of the possi
ble integro-differential evolution equations has a cubic-nonlinearity
due to supercriticality (non-neutrality) effects, while the other ampl
itude evolution equation has a quintic nonlinearity but is only releva
nt for larger sizes of disturbance. Thus, in this paper, attention is
concentrated on the former, since this equation is appropriate earlier
in the evolution process of the Gortler modes, Numerical results are
presented which demonstrate that variations in the level of cross-flow
present in the underlying flow have a significant effect on the nonli
near problem, as the!: do on the linear problem. It is: found that the
consideration of a spatial evolution problem (as opposed to a tempora
l stability approach adopted in the above paper) leads to significant
changes to the resulting evolution equations.